Newton's Principia : $b The mathematical principles of natural philosophyNewton, Isaac
General
Newton's Principia : $b The mathematical principles of natural philosophy
Newton, Isaac
Celestial mechanics -- Early works to 1800; Mechanics -- Early works to 1800
The last construction remaining, let the body T go from the given
place S, in the direction of a line given by position, and turn into
the trajectory sought STR, whose orthographic projection in the plane
BDO is AP. And from the given velocity of the body in the altitude SC,
its velocity in any other altitude TC will be also given. With that
velocity, in a given moment of time, let the body describe the particle
Tt of its trajectory, and let Pp be the projection of
that particle described in the plane AOP. Join Op, and a little
circle being described upon the curve superficies about the centre T[Pg 194]
with the interval Tt let the projection of that little circle in
the plane AOP be the ellipsis pQ. And because the magnitude of
that little circle Tt, and TN or PO its distance from the axis
CO is also given, the ellipsis pQ will be given both in kind
and magnitude, as also its position to the right line PO. And since
the area POp is proportional to the time, and therefore given
because the time is given, the angle POp will be given. And
thence will be given p the common intersection of the ellipsis
and the right line Op, together with the angle OPp, in
which the projection APp of the trajectory cuts the line OP.
But from thence (by conferring Prop. XLI, with its 2d Cor.) the manner
of determining the curve APp easily appears. Then from the
several points P of that projection erecting to the plane AOP, the
perpendiculars PT meeting the curve superficies in T, there will be
given the several points T of the trajectory. Q.E.I.
SECTION XI.
Of the motions of bodies tending to each other with centripetal
forces.
I have hitherto been treating of the attractions of bodies towards an
immovable centre; though very probably there is no such thing existent
in nature. For attractions are made towards bodies, and the actions of
the bodies attracted and attracting are always reciprocal and equal,
by Law III; so that if there are two bodies, neither the attracted
nor the attracting body is truly at rest, but both (by Cor. 4, of the
Laws of Motion), being as it were mutually attracted, revolve about a
common centre of gravity. And if there be more bodies, which are either
attracted by one single one which is attracted by them again, or which
all of them, attract each other mutually, these bodies will be so moved
among themselves, as that their common centre of gravity will either be
at rest, or move uniformly forward in a right line. I shall therefore
at present go on to treat of the motion of bodies mutually attracting
each other; considering the centripetal forces as attractions; though
perhaps in a physical strictness they may more truly be called
impulses. But these propositions are to be considered as purely
mathematical; and therefore, laying aside all physical considerations,
I make use of a familiar way of speaking, to make myself the more
easily understood by a mathematical reader.
PROPOSITION LVII. THEOREM XX.
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